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Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
机构
过程工程研究所 [1]
高能物理研究所 [1]
沈阳应用生态研究所 [1]
合肥物质科学研究院 [1]
采集方式
OAI收割 [4]
内容类型
期刊论文 [4]
发表日期
2021 [1]
2018 [2]
2016 [1]
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Antisaturation Finite-Time Attitude Tracking Control Based Observer for a Quadrotor
期刊论文
OAI收割
IEEE TRANSACTIONS ON CIRCUITS AND SYSTEMS II-EXPRESS BRIEFS, 2021, 卷号: 68
作者:
Liu, Kang
;
Wang, Xingxian
;
Wang, Rujing
;
Sun, Guowei
;
Wang, Xiaodong
  |  
收藏
  |  
浏览/下载:46/0
  |  
提交时间:2021/08/31
Observers
Symmetric matrices
Convergence
Attitude control
Angular velocity
Circuits and systems
Manifolds
Attitude control
extended state observer
fast nonsingular terminal sliding mode
wind disturbance
Usefulness of multi-solids pneumatic transport bed data for evaluation and validation of binary solids computational simulation models
期刊论文
OAI收割
POWDER TECHNOLOGY, 2018, 卷号: 327, 页码: 70-78
作者:
Liu, Wenming
;
Bi, Xiaotao T.
;
Zhu, Qingshan
;
Li, Hongzhong
  |  
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2018/06/11
Fluidization
Coarse Particle Terminal Velocity
Fine Particle Holdup
Binary Mixture
A New Set of Parameters of High-Mass X-ray Binaries Found with their Cyclotron Lines
期刊论文
OAI收割
arXiv e-prints, 2018
作者:
Zhang, Chengmin
;
Taani, Ali
;
Chaty, Sylvain
;
Karino, Shigeyuki
;
Song, Liming
  |  
收藏
  |  
浏览/下载:76/0
  |  
提交时间:2019/07/12
Astrophysics - High Energy Astrophysical Phenomena
Abstract: We have derived new physical quantities for several High-Mass X-ray Binaries (HMXBs) with supergiant (SG) companions through their cyclotron lines. The parameters are: the terminal velocity of the wind, the mass loss rate of the donor, the effective temperature and the magnetic fields. These parameters influence significantly the improvement of the model of accretion. In spite of the variety of their observational properties, the corresponding magnetic field is around B ~ 10^12 G. This result can be constrained by the effects on stellar evolution. In addition, we have performed a segmentation in the parameter space of donors intended for several SG-HMXB listed in our sample set. The parameter space can be categorized into five regimes depending on the possibility of disk formation associated with accretion from the stellar wind. This can give a quantitative clarification of the observed variability and the properties of these objects. We show that, when these systems come into the direct accretion region, systems with corresponding parameters can emit X-rays.
Which factors have stronger explanatory power for primary wind dispersal distance of winged diaspores: the case of Zygophyllum xanthoxylon (Zygophyllaceae)?
期刊论文
OAI收割
JOURNAL OF PLANT ECOLOGY, 2016, 卷号: 9, 期号: 3, 页码: 346-356
作者:
Zhu, Jinlei
;
Liu, Minghu
;
Xin, Zhiming
;
Zhao, Yingming
;
Liu, Zhimin
  |  
收藏
  |  
浏览/下载:27/0
  |  
提交时间:2019/06/04
Zygophyllum Xanthoxylon (Zygophyllaceae)
Seed Dispersal By Wind
Seed Morphology
Terminal Velocity
Wind Tunnel Experiment